“…Furthermore, in [13,14] in the MPCM with tensor forces the possibility of the correct reproduction practically of all characteristics of 6 Li was demonstrated, including its quadrupole momentum. Subsequently, in [15][16][17][18] on the basis of the MPCM we have presented the possibility of description of the astrophysical S-factors or the total cross sections of almost 30 radiative capture processes, namely, p 2 H, n 2 H, p 3 H, p 6 Li, n 6 Li, p 7 Li, n 7 Li, p 9 Be, n 9 Be, p 10 B, n 10 B, p 11 B, n 11 B, p 12 C, n 12 C, p 13 C, n 13 C, p 14 C, n 14 C, n 14 N, p 15 N, n 15 N, n 16 O and 2 H 4 He, 3 He 4 He, 3 H 4 He, 4 He 12 C systems at thermal and astrophysical energies (see also [2][3][4][5][6][7]). Continuing study of thermonuclear reactions in the frame of the modified potential cluster model with forbidden states [15][16][17][18] let us consider the 16 O(p,) 17 F process, which takes part of the CNO cycle [15,16] and has additional interest, since it is the reaction at the last nucleus of 1p-shell with the forming of 17 F that get out its limit.…”